Venus will reach half phase in its 2018 evening apparition. It will be shining brightly at mag -4.3.
2018 evening apparition of Venus
|09 Jan 2018||–||Venus at superior solar conjunction|
|13 Jun 2018||–||Venus at highest altitude in evening sky|
|15 Aug 2018||–||Venus at dichotomy|
|17 Aug 2018||–||Venus at greatest elongation east|
|25 Sep 2018||–||Venus at greatest brightness|
The table below lists the altitude of Venus at sunset over the course of the apparition. All times are given in Ashburn local time.
|15 Mar 2018||19:18||20:28||13°||west||-3.9||96%|
|25 Mar 2018||19:27||20:52||15°||west||-3.9||95%|
|04 Apr 2018||19:39||21:16||17°||west||-3.9||94%|
|14 Apr 2018||19:48||21:39||20°||west||-3.9||92%|
|24 Apr 2018||19:57||22:03||22°||west||-3.9||90%|
|04 May 2018||20:07||22:24||24°||west||-3.9||88%|
|14 May 2018||20:18||22:43||25°||west||-4.0||85%|
|24 May 2018||20:26||22:58||26°||west||-4.0||83%|
|03 Jun 2018||20:31||23:07||27°||west||-4.0||80%|
|13 Jun 2018||20:36||23:08||27°||west||-4.0||76%|
|23 Jun 2018||20:42||23:09||27°||west||-4.0||73%|
|03 Jul 2018||20:39||22:59||26°||west||-4.1||69%|
|13 Jul 2018||20:36||22:49||25°||west||-4.1||65%|
|23 Jul 2018||20:32||22:34||23°||west||-4.2||61%|
|02 Aug 2018||20:23||22:14||21°||west||-4.2||56%|
|12 Aug 2018||20:10||21:58||20°||west||-4.3||52%|
|22 Aug 2018||19:59||21:34||17°||south-west||-4.4||46%|
|01 Sep 2018||19:43||21:14||15°||south-west||-4.4||40%|
Altitude of Venus at sunset
A graph of the phase of Venus is available here.
Apparitions of Venus
|26 Oct 2015||–||Morning apparition|
|12 Jan 2017||–||Evening apparition|
|03 Jun 2017||–||Morning apparition|
|17 Aug 2018||–||Evening apparition|
|06 Jan 2019||–||Morning apparition|
|24 Mar 2020||–||Evening apparition|
|13 Aug 2020||–||Morning apparition|
Venus's orbit lies closer to the Sun than the Earth's, meaning that it always appears close to the Sun and is lost in the Sun's glare much of the time.
It is observable for a few months each time it reaches greatest separation from the Sun – moments referred to as greatest elongation. These apparitions repeat roughly once every 1.6 years.
On these occasions, Venus is so bright and conspicuous that it becomes the third brightest object in the sky after the Sun and Moon. It is often called the morning star or the evening star.
Venus's phase varies depending on its position relative to the Earth. When it passes between the Earth and Sun, for example, the side that is turned towards the Earth is entirely unilluminated, like a new moon.
Conversely, when it lies opposite to the Earth in its orbit, passing almost behind the Sun, it appears fully illuminated, like a full moon. However, at this time it is also at its most distant from the Earth, so it is actually fainter than at other times.
Venus shows an intermediate half phase – called dichotomy – at roughly the same moment that it appears furthest from the Sun, at greatest elongation. The exact times of the two events may differ by a few days, only because Venus's orbit is not quite perfectly aligned with the ecliptic.
The coordinates of Venus when it reaches dichotomy will be:
|Object||Right Ascension||Declination||Constellation||Angular Size|
The coordinates above are given in J2000.0.
|The sky on 15 August 2018|
4 days old
All times shown in EDT.
The circumstances of this event were computed using the DE430 planetary ephemeris published by the Jet Propulsion Laboratory (JPL).
This event was automatically generated by searching the ephemeris for planetary alignments which are of interest to amateur astronomers, and the text above was generated based on an estimate of your location.
|15 Aug 2018||– Venus at dichotomy|
|17 Aug 2018||– Venus at greatest elongation east|
|05 Sep 2018||– Venus at aphelion|
|25 Sep 2018||– Venus at greatest brightness|
© NASA/Ricardo Nunes